Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351
Fuente:
arXiv
Salvato in:
| Autori principali: | , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Natura: | Preprint |
| Pubblicazione: |
2026
|
| Soggetti: | |
| Accesso online: | |
| Tags: |
Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
|
| _version_ | 1866912980665368576 |
|---|---|
| author | Srikanth, K. S. L. Botteon, A. Cassano, R. Brunetti, G. Bonafede, A. Bruno, L. Balboni, M. Bashir, H. Brüggen, M. Chatterjee, S. Cuciti, V. Dallacasa, D. Datta, A. de Gasperin, F. Di Gennaro, G. Groeneveld, C. Kale, R. Malik, M. A. Paul, S. Salunkhe, S. van Weeren, R. J. Venturi, T. Zhang, X. |
| author_facet | Srikanth, K. S. L. Botteon, A. Cassano, R. Brunetti, G. Bonafede, A. Bruno, L. Balboni, M. Bashir, H. Brüggen, M. Chatterjee, S. Cuciti, V. Dallacasa, D. Datta, A. de Gasperin, F. Di Gennaro, G. Groeneveld, C. Kale, R. Malik, M. A. Paul, S. Salunkhe, S. van Weeren, R. J. Venturi, T. Zhang, X. |
| contents | Radio halos are megaparsec-scale diffuse, non-thermal radio sources located at the centers of galaxy clusters, tracing relativistic particles and magnetic fields in the intra-cluster medium. Their origin is generally attributed to cluster mergers that generate turbulence and re-accelerate aged electrons. We study the diffuse radio emission, spectral properties, and the connection between thermal and non-thermal components in the massive galaxy clusters Abell 773 and Abell 1351 ($M_{500} \sim 7 \times 10^{14}\,M_{\odot}$), both of which are dynamically disturbed. We combine LOFAR LoTSS-DR2 observations at 144 MHz with uGMRT observations at 650 MHz, supplemented by archival XMM-Newton X-ray imaging. We confirm that both clusters host radio halos extending up to a largest linear size of $\sim 2$ Mpc. We measure an integrated spectral index $α_{144}^{650} \sim -1.0$ for both clusters. The radio halo in Abell 773 resembles a classical halo and follows a sublinear radio--X-ray surface brightness relation. In contrast, Abell 1351 shows a more complex and asymmetric morphology, influenced by embedded radio sources including the brightest cluster galaxy, a tailed radio galaxy, and a ridge-like feature. These contaminating sources lead to deviations from the sublinear trend in the point-to-point radio--X-ray analysis of Abell 1351. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2601_13316 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351 Srikanth, K. S. L. Botteon, A. Cassano, R. Brunetti, G. Bonafede, A. Bruno, L. Balboni, M. Bashir, H. Brüggen, M. Chatterjee, S. Cuciti, V. Dallacasa, D. Datta, A. de Gasperin, F. Di Gennaro, G. Groeneveld, C. Kale, R. Malik, M. A. Paul, S. Salunkhe, S. van Weeren, R. J. Venturi, T. Zhang, X. Cosmology and Nongalactic Astrophysics Radio halos are megaparsec-scale diffuse, non-thermal radio sources located at the centers of galaxy clusters, tracing relativistic particles and magnetic fields in the intra-cluster medium. Their origin is generally attributed to cluster mergers that generate turbulence and re-accelerate aged electrons. We study the diffuse radio emission, spectral properties, and the connection between thermal and non-thermal components in the massive galaxy clusters Abell 773 and Abell 1351 ($M_{500} \sim 7 \times 10^{14}\,M_{\odot}$), both of which are dynamically disturbed. We combine LOFAR LoTSS-DR2 observations at 144 MHz with uGMRT observations at 650 MHz, supplemented by archival XMM-Newton X-ray imaging. We confirm that both clusters host radio halos extending up to a largest linear size of $\sim 2$ Mpc. We measure an integrated spectral index $α_{144}^{650} \sim -1.0$ for both clusters. The radio halo in Abell 773 resembles a classical halo and follows a sublinear radio--X-ray surface brightness relation. In contrast, Abell 1351 shows a more complex and asymmetric morphology, influenced by embedded radio sources including the brightest cluster galaxy, a tailed radio galaxy, and a ridge-like feature. These contaminating sources lead to deviations from the sublinear trend in the point-to-point radio--X-ray analysis of Abell 1351. |
| title | Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351 |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2601.13316 |